Budget Woes Put SETI’s Allen Telescope Array into “Hibernation”

Allen Telescope Array. Credit: ATA

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SETI, the Search for Extraterrestrial Intelligence has suffered a big blow. The primary alien search engine –the Allen Telescope Array (ATA) in northern California — has been shut down due to budget woes. In a letter last week, the CEO of the SETI Institute, Tom Pierson told donors that in the ATA has been put into “hibernation,” — a safe mode of sorts, where “the equipment is unavailable for normal observations and is being maintained in a safe state by a significantly reduced staff.”

The ATA has been in hibernation since April 15, with the equipment put in a safe configuration so that it stays ready to be turned back on should the SETI Institute find new sources of funding.

While the ATA is not the only radio telescope that can be used for SETI searches, it was the observatory that was primarily used for that task, and now SETI researchers will have to borrow time on telescopes where “competition for observing time can be fierce or piggyback their searches on other ongoing observations,” according to John Matson, writing for Scientific American.

The ATA was operating with 42 antennas, and was scheduled to expand gradually to 350 six-meter radio antennas to listen for possible radio emissions from any faraway civilizations that might exist elsewhere in the galaxy. But after the first $50 million phase was completed in 2007, additions to the array were delayed due to lack of funding.

NASA had funded some of the early SETI projects, but Congress canceled any NASA contributions in 1993. The nonprofit SETI Institute, founded in 1984, relies mainly on private donations to support its research. Microsoft co-founder Paul Allen, had contributed $25 million to the first phase, with donations and grants funding the rest.

According to astronomer Franck Marchis, who works for the SETI Institute and the University of California, Berkeley – which is responsible for operating the ATA, “the financial state of the observatory degraded significantly over the past 2 years with the loss of various sources of funding (NSF, California state) at UC Berkeley” forcing UC Berkeley to withdraw from the SETI project. And, as Marchis wrote on his blog, “because the project is mainly funded through private donors, the economic recession had a huge impact and delayed significantly the expansion of the array impacting the overall project.”

In his letter, Pierson said that NSF funding has been reduced to approximately one-tenth of what it formerly gave to SETI. “This is compounded by growing State of California budget shortfalls that have severely reduced the amount of state funds available to the Radio Astronomy Lab.”

ATA operations cost about $1.5 million per year, Pierson said, and the SETI science campaign at ATA costs another $1 million annually.

Pierson said that the SETI Institute has been working for more than two years to find additional funding, such as providing assistance to the US Air Force in tracking orbital debris. The SETI Institute is also currently working on a fundraising campaign to raise $5 million so that the ATA can be used to focus on the potentially habitable planets found by the Kepler telescope.

For anyone who is interested in donating SETI, and in particular the ATA and their search of signals from the Kepler database of planets, see this website.

Sources: Scientific American, Cosmic Diary, SETI Institute

“Astrobiology” Parody Video of Ke$ha’s “We R Who We R”

Wanna get turned on by … “Astrobiology” ?? Are we alone in the universe?

Well check out just this newly-released music video parody of Ke$ha’s hit song “We R Who We R” – “Astrobiology.”

Suspend your disbelief. It’s different. It’s cool. And it’s very clever.

And .. It’s even better the second time around when you listen to the lyrics more closely … combined with the shocking video .. Featuring beautiful maidens and alien dolls galore. Continue reading ““Astrobiology” Parody Video of Ke$ha’s “We R Who We R””

Buzz About Gliese 581g: Doubts of Its Existence; Aliens Signals Detected

Goldilocks Zone
Artists impression of Gliese 581g. Credit: Lynette Cook/NSF

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Ever since the announcement of the discovery of exoplanet Gliese 581g, there has been a buzz in the news, on websites, Twitter – pretty much everywhere, about the first potentially habitable extrasolar planet. But the past couple of days there has been a different sort of buzz about this distant world. Two stories have surfaced and they both can’t be true. The first one is fairly off the deep end: an astrophysicist from Australia claims that while doing a SETI search two years ago, he picked up a “suspicious signal” from the vicinity of the Gliese 581 system, and a couple of websites have connected some dots between that signal and a potentially habitable Gliese 581g.

The second one is more sobering. At an International Astronomical Union meeting this week, other astronomers have raised doubts whether Gliese 581g actually exists.

Unless you’ve been under a rock the past two weeks, you likely know that this newest and most promising of potential habitable extra solar planets was described by the scientists who discovered it as a rocky world about 3 times the mass of Earth, and it orbits within the red dwarf star’s habitable zone, the place that is just right for water to remain as a liquid on a planetary surface. And it is fairly close to us, too, at about 20 light years away, located in the constellation Libra.

Also announced was the discovery of planet ‘f’, a 7-Earth mass planet with a 433-day orbit around Gliese 581.

Astronomer Steven Vogt announced the discoveries by his team, which used the HIRES instrument on the Keck I telescope in Hawaii. They also used 119 measurements from the HARPS instrument on the La Silla telescope at the European Southern Observatory in Chile.

On Monday, Steinn Siggurdson broke the news on his Dynamics of Cats blog that an astronomer who works on HARPS data at the Geneva Observatory, said at the IAU meeting this week that his team could not confirm the existence of Gliese 581 g.

In an article on the Astrobiology Magazine website today (Tuesday) the astronomer, Francesco Pepe, said that not only can they not confirm the existence of planet ‘g’, but also the ‘f’ planet.

In 2009, the Geneva team announced the discovery of planet ‘e’ in the Gliese 581 solar system. At approximately 1.9 Earth masses, this ‘e’ planet is the lowest mass extrasolar planet found at that time, and has a 3.15-day orbital period around the star.

Pepe said they have studied this planet-rich system frequently, gathering a total of 180 data points in 6.5 years (with about 60 of those data points since 2009) and they can only see evidence of the 4 previously announced planets b, c, d, and e.

There is a signal which could possibly be f, but the signal amplitude of this potential fifth planet is very low and basically at the level of the measurement noise, said Pepe.

The planets in the Gliese 581 system were discovered using spectroscopic radial velocity measurements. Planets ‘tug’ on the star they orbit, causing it to shift in position (stars and planets actually orbit a common center of mass). By measuring the star’s movement in the sky, astronomers can figure out what sort of planets are orbiting it. Multi-planet systems create a complicated signal, and astronomers must tease out the spectral lines to figure out what represents a planet, and what is just “noise” – shifts in the star light not caused by an orbiting planet. Astronomers have developed various ways to reduce such noise in their telescopic observations, but it still creates a level of uncertainty in detecting extrasolar planets.

The Geneva team plugged the HARPS data on Gliese 581 into computer models, and the models show “the probability that such a signal is just produced ‘by chance’ out of the noise is not negligible, of the order of several percents,” Pepe said. “Under these conditions we cannot confirm the presence of the announced planet Gliese 581 g.”

While this doesn’t definitively mean Gliese 581g doesn’t exist, it certainly casts doubt on it. More teams will be looking at the Gliese 581 star to try and determine what is really out there. This story is not over yet.

As for the alien signal, this news has met some pretty harsh criticism — even from Dr. Frank Drake, a leader in SETI community. Astronomer Ragbir Bhathal, a scientist at the University of Western Sydney, said he detected an unusual pulse of light nearly two years ago from the same region at Gliese 581, and with the news of the potential habitable world there, his claims came up again. In an article in Space.com Drake said is suspicious because Bhathal would not share his data with anyone.

You can read an article published in 2009 in the Australian about Bhathal’s claimed discovery.

Watch SETI Webcast This Week

The National Radio Astronomy Observatory (NRAO) is sponsoring a workshop this week on the past and next 50 years of SETI (Search for Extraterrestrial Intelligence) an (SETI), and they are webcasting many of the sessions on Monday, Tuesday and Wednesday of this week, September 13-15. The workshop featuring leading scientific researchers as well as authors, historians, religious leaders, and biologists. Viewers will be able to send questions to the presenters. The webcasts begin at 8:30 a.m., EDT, on September 13, 14, and 15, and can be watched above, or at this link.

You can see the workshop schedule at this link.

Drake will webcast his views on “SETI in 2061 and Beyond”, at 8:30 a.m., EDT, on September 15.

“This workshop focuses on a topic that has a profound influence on the way we view ourselves and our place in the Universe,” said Dr. Glen Langston, NRAO astronomer and workshop organizer. “We are pleased to present this to the public through the webcast.”

Maybe ET’s Calling, But We Have the Wrong Phone

The search (xkcd)

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To date, SETI (Search for ExtraTerrestrial Intelligence) has focused on ETs who ‘phone home’ using the radio part of the electromagnetic spectrum, and even a very small region within that.

But what if ET’s phone doesn’t use radio waves? Sure the xkcd comic, is funny, but maybe it points to a deep flaw in our attempts to contact, or hear from, an ETI?

When Giuseppe Cocconi and Philip Morrison suggested the possibility of interstellar communication via electromagnetic waves in a 1959 paper in Nature, only radio was feasible, as we then had the ability to detect only artificial radio signals, if produced by ETIs with 1959 human technology. Since then we’ve developed the ability to detect a laser signal, brighter than the Sun (if only for a nanosecond) if it came from a source several light-years away … but lasers weren’t invented then.

What might ET’s equivalent of ants’ pheromones be?

Back in 1959 if you’d said that the Earth would, within a mere half century, started to go ‘radio quiet’, not many people would have taken you seriously. Yet that’s exactly what’s happened! Free to air (FTA) broadcasting, especially for TV, is being replaced by TV delivered over coaxial cable, optical fibers, or even the phone company’s twisted copper pairs. And where it’s continuing, as in satellite TV broadcasting, its power has dropped (today’s digital formats are more efficient than the old analog ones). Military radars, the brightest source of artificial radio waves by far, no longer broadcast in a single channel, but hop, rapidly, from frequency to frequency, to avoid jamming.

“Our improving technology is causing the Earth to become less visible,” says astronomer Frank Drake, SETI’s paterfamilias. “If we are the model for the universe, that is bad news.”

In the past half century SETI researchers have expanded the scope of their searches. Not only are far more radio channels being examined, but artificial signals in the optical are being sought too. How to decide which of the billions or trillions of possible radio channels to search? For example, the Allen Telescope Array will, when built, monitor a billion channels between 0.5 and 11 GHz – but that’s a trivial fraction of the entire radio waveband. Some ideas, however, seem cute; for example, the SETI Institute’s Gerald Harp has proposed searching at 4.462336275 gigahertz, in what’s called the PiHI range, because it’s the hydrogen atom’s emission frequency times pi. More seriously, Harvard University’s Paul Horowitz says optical SETI programs should really look at infrared frequencies “Stars are darker in the infrared and lasers are brighter and the smog goes away,” Horowitz says. Infrared allows astronomers to see into the galactic center, where dust scatters visible light.

There’s something rather ironic about SETI today; on the one hand, we recognize that our initial hopes were far too high, being based on overly simplistic assumptions; on the other, the tremendous progress in finding exoplanets has given us greater and greater certainty that Earth-like planets not only exist, but are, very likely, common. “All of astronomy has come to embrace this idea that there must be life out there,” says Harp.

So how to address the fact that we simply do not know what sorts of technologies a civilization like ours may have, a century or a millennium from now? After all, as Drake says “We are very conservative at SETI, we assume in our searches the existence of only things we ourselves have and know how to make.” Other scientists, and SETI enthusiasts, have proposed hunting in different electromagnetic realms, like gamma rays. Spacecraft that rely on nuclear fusion or antimatter-matter annihilation as a power source might produce such rays. But standard SETI strategy does not embrace such “speculative” scenarios.

SETI researchers, some say, should also contemplate what technologies supersmart aliens might possess and seek out the corresponding signals. In a 2008 arXiv paper, “Galactic Neutrino Communication“, John Learned of the University of Hawaii at Manoa suggested that ET could be sending beams of neutrinos Earth’s way. Energy requirements for such a beam make that scenario seem implausible, but not necessarily impossible. Detectors currently under construction, such as IceCube at the South Pole, could spot unexpected stray neutrinos. If a few with the same energy came from the same direction, astronomers would know something screwy was up.

In another paper, “The Cepheid Galactic Internet“, Learned suggests that ET could send a signal using a neutrino beam to deliver energy to a Cepheid variable. A Cepheid “blows up and comes crashing back down,” he says. “And the energy builds up and it blows again, like a geyser.” ET could leverage a Cepheid’s inherent instability by delivering a boost of energy that messes with the star’s schedule. Looking through existing data could reveal whether such meddling has occurred. “All that is needed is people analyzing for other reasons to do their analyses in another way,” Learned says.

Drake and most others agree that SETI’s approach should be multidirectional – let a thousand alien hunters bloom. The only ideas that don’t do anybody any good, Horowitz says, are the ones for which there is no conceivable way to look. “I’d like to keep an open mind,” he says, “but not so much that my brain falls out.”

Physicist Paul Davies of Arizona State University in Tempe, however, suggests that researchers don’t need to know what to look for. Find the fishy thing first, and then argue about its origin, he says.

As Davies has argued, maybe discovering ET does indeed depend on a thought revolution. Fifty years of signal-less searching suggests that the problem could lie not with the aliens among the stars, but with ourselves.

Maybe the sentient ants should not give up, just yet.

Sources: Science News. Cocconi and Morrison’s 1959 Nature paper (copyright Nature)

Astronomy Without A Telescope – SETI 2.0

Allen Telescope Array. Credit: SETI Institute

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Fifty years of eerie silence in the search for extra-terrestrial intelligence has prompted some rethinking about what we should be looking for.

After all, it’s unlikely that many civilizations would invest a lot of time and resources into broadcasting a Yoo-hoo, over here signal, so maybe we have to look for incidental signs of alien activity – anything from atmospheric pollution on an exoplanet to signs of stellar engineering undertaken by an alien civilization working to keep their aging star from turning into a red giant.

We know a spectroscopic analysis of Earth’s atmosphere will indicate free molecular oxygen – a tell tale sign of life. The presence of chlorofluorocarbons would also be highly suggestive of advanced industrial activity. We also know that atomic bomb tests in the fifties produced perturbations to the Van Allen belts that probably persisted for weeks after each blast.

These are planet level signs of a civilization still below the level of a Kardashev Type 1 civilization. We are at level 0.73 apparently. A civilization that has reached the Type 1 level is capable of harnessing all the power available upon a single planet – and might be one that inadvertently signals its presence after thoughtfully disposing of large quantities of nuclear waste in its star. To find them, we should be scanning A and F type stars for spectral signatures of technetium – or perhaps an overabundance of praseodymium and neodymium.

We might also look for signs of stellar engineering indicative of a civilization approaching the Kardashev Type 2 level, which is a civilization able to harness all the power of a star. Here, we might find an alien civilization in the process of star lifting, where an artificial equatorial ring of electric current creates a magnetic field sufficient to both increase and deflect all the star’s stellar wind into two narrow polar jets.

Left image - A proposed model for 'star lifting'. An artificial equatorial ring of electric current (RC) produces a magnetic field which enhances and directs the star's stellar wind though magnetic nozzles (MN) to produce two polar jets (J). Right image (Credit: SETI institute) - Artists impression of the completed Allen Telescope Array for future SETI observations. The lead image for this article is part of the current Allen Array prototype, comprising 42 of the proposed 350 dishes.

These jets could be used for power generation, but might also represent a way to prolong the life of an aging star. Indeed, this may become a vital strategy for us to prolong the solar system’s habitable zone at Earth’s orbit. In less than a billion years, Earth’s oceans are expected to evaporate due to the Sun’s steadily increasing luminosity, but some carefully managed star lifting to modify the Sun’s mass could extend this time limit significantly.

It’s also likely that Type 2 civilizations will play with Hertzsprung–Russell (H-R) parameters to keep their Sun from evolving onto the red giant branch of the H-R diagram – or otherwise from going supernova. Some well placed and appropriately shielded nuclear bombs might be sufficient to stir up stellar material that would delay a star’s shift to core helium fusion – or otherwise to core collapse.

It’s been hypothesized that mysterious giant blue straggler stars, which have not gone supernova like most stars of their type would, may have been tinkered with in this manner (some stress on the word hypothesized there).

As for detecting Type 3 civilizations… tricky. It’s speculated that they might build Dyson nets around supermassive black holes to harvest energy at a galactic level. But indications are that they then just use all that energy to go around annoying the starship captains of Type I civilizations. So, maybe we need to draw a line about who exactly we want to find out there.

Further reading:

Starry Messages: Searching for Signatures of Interstellar Archaeology http://arxiv.org/abs/1001.5455

Detectability of Extraterrestrial Technological Activities http://www.coseti.org/lemarch1.htm

If the Earth is Rare, We May Not Hear from ET

Earth - Moon System
Image Credit: NASA

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If civilization-forming intelligent life is rare in our Milky Way galaxy, chances are we won’t hear from ET before the Sun goes red giant, in about five billion years’ time; however, if we do hear from ET before then, we’ll have lots of nice chats before the Earth is sterilized.

That’s the conclusion from a recent study of Ward and Brownlee’s Rare Earth hypothesis by Duncan Forgan and Ken Rice, in which they made a toy galaxy, simulating the real one we live in, and ran it 30 times. In their toy galaxy, intelligent life formed on Earth-like planets only, just as it does in the Rare Earth hypothesis.

While the Forgan and Rice simulations are still limited and somewhat unrealistic, they give a better handle on SETI’s chances for success than either the Drake equation or Fermi’s “Where are they?”

“The Drake equation itself does suffer from some key weaknesses: it relies strongly on mean estimations of variables such as the star formation rate; it is unable to incorporate the effects of the physico-chemical history of the galaxy, or the time-dependence of its terms,” Forgan says, “Indeed, it is criticized for its polarizing effect on “contact optimists” and “contact pessimists”, who ascribe very different values to the parameters, and return values of the number of galactic civilizations who can communicate with Earth between a hundred-thousandth and a million (!)”

Building on the work of Vukotic and Cirkovic, Forgan developed a Monte Carlo-based simulation of our galaxy; as inputs, he used the best estimates of actual astrophysical parameters such as the star formation rate, initial mass function, a star’s time spent on the main sequence, likelihood of death from the skies, etc. For several key inputs however, “the model goes beyond relatively well-constrained parameters, and becomes hypothesis,” Forgan explains, “In essence, the method generates a Galaxy of a billion stars, each with their own stellar properties (mass, luminosity, location in the Galaxy, etc.) randomly selected from observed statistical distributions. Planetary systems are then generated for these stars in a similar manner, and life is allowed to evolve in these planets according to some hypothesis of origin. The end result is a mock Galaxy which is statistically representative of the Milky Way. To quantify random sampling errors, this process is repeated many times: this allows an estimation of the sample mean and sample standard deviation of the output variables obtained.”

Forgan simulated the Rare Earth hypothesis by allowing animal life – the only kind of life from which intelligent civilizations can arise – to form only if homeworld’s mass is between a half and two Earths, if homesun’s mass is between a half and 1.5 times our Sun’s, homeworld has at least one moon (for tides and axial stability), and if homesun has at least one planet of mass at least ten times that of Earth, in an outer orbit (to cut down on death from the skies due to asteroids and comets).

The good news for SETI is that a galaxy like ours should host hundreds of intelligent civilizations (though, somewhat surprisingly, there is no galactic goldilocks zone); the bad news is that during the time such a civilization could communicate with an ET – between when it becomes technologically advanced enough and when it is wiped out by homesun going red giant – there are, in most simulations, no other such civilizations (or if there are, they are too far away) … we, or ET, would be alone.

But it’s not all bad news; if we are not alone, then once contact is established, we will have many phone calls with ET.

To be sure, this is but a work-in-progress. “Numerical modeling of this type is generally a shadow of the entity it attempts to model, in this case the Milky Way and its constituent stars, planets and other objects,” Forgan and Rice say; several improvements are already being worked on.

Sources: “A numerical testbed for hypotheses of extraterrestrial life and intelligence” (Forgan D., 2009, International Journal of Astrobiology, 8, 121), and “Numerical Testing of The Rare Earth Hypothesis using Monte Carlo Realisation Techniques” (arXiv:1001:1680); this too will be published in IJA, likely in April.

So Where Is ET, Anyway?

While having lunch with colleagues at Los Alamos National Labs in 1950, physicist Enrico Fermi mused about the likelihood of intelligent life existing elsewhere in the Universe.  Fermi, one of the most astute scientists of his day, thought the size and age of the Universe means many advanced civilizations should have already colonized the galaxy, just as humans colonized and explored the Earth.   But if such galaxy-wide extraterrestrial civilizations exist, he wondered, where are they?

Some believe this problem, called the Fermi Paradox, means advanced extraterrestrial societies are rare or nonexistent.  Others suggest they must destroy themselves before they move on to the stars.

But this week, Jacob D. Haqq-Misra and Seth D. Baum at Penn State University proposed another solution to the Fermi Paradox: that extraterrestrial civilizations haven’t colonized the galaxy because the exponential growth of a civilization required to do so is unsustainable.

The researchers call their idea the “Sustainability Solution”.  It states: “The absence of ETI (extra-terrestrial intelligence) observation can be explained by the possibility that exponential or other faster growth is not a sustainable development pattern for intelligent civilizations.”

The researchers base their conclusions on a study of civilizations on Earth.  Historically, rapid growth of societies means rapid resource depletion and environmental degradation, usually with dire results.  They cite the example of Easter Island, where resource depletion likely caused a collapse of the local population.  And they conclude that while there are examples of sustainable growth like the !Kung San people of the Kalahari Desert, exponential growth in population and spatial expansion of a society is almost always linked to unsustainable growth and eventual collapse.

This principle has implications for our current global civilization.  Since Earth’s resources are finite and it receives solar radiation at a constant rate, human civilization cannot sustain an indefinite, exponential growth.  But even if we survive and advance as a civilization, we may have trouble colonizing the galaxy should we ever decide to do so.  And if this limitation applies to us, it may apply to other civilizations as well.

But the Sustainability Solution doesn’t mean ET is not out there.  Slower-growth extraterrestrial societies might still communicate by radio or other wavelengths, so current SETI programs still make sense.  Or ETI may result in chemical bio-markers in planetary atmospheres which may leave spectroscopic signatures detectable with upcoming generations of Earth and space-based planet-hunting telescopes.

The Sustainability Solution also allows that advanced civilizations may indeed colonize the galaxy, then collapse as resources are consumed at an unsustainable rate.

And some civilizations may send small messenger probes to other stars, which suggests a search for extraterrestrial artifacts (SETA) within our own solar system might be just as fruitful as radio-based SETI.  Searches might involve radio or visible detection of extraterrestrial probes orbiting the sun.  Or artifacts may even be embedded within planets or moons of our solar system, just like the giant black monoliths in Arthur C. Clarke’s 2001: A Space Odyssey.

In any case, the discovery of artifacts from a slow-growth extraterrestrial civilization would be an example “sustainable development” on a galactic scale.

You can read the original article here.

A New Drake Equation? Other Life Not Likely to be Intelligent

Radio Telescopes. Credit: University of Washington

Looking for signals from distant civilizations might be an effort in futility, according to scientists who met at Harvard University recently. The dominant view of astronomers at a symposium on the future of human life in the Universe seems to be that if other life is out there, it likely is dominated by microbes or other nonspeaking creatures.

Speakers reviewed how life on Earth arose and the many, sometimes improbable steps it took to create intelligence here. Radio astronomer Gerrit Verschuur said he believes that though there is very likely life out there — perhaps a lot of it — it is very unlikely to be both intelligent and able to communicate with us.

Verschuur presented his take on the Drake equation, formulated by astronomer Frank Drake in 1960, that provides a means for calculating the number of intelligent civilizations that it is possible for humans to make contact with.

The equation relates those chances to the rate of star and habitable planet formation. It includes the rate at which life arises on such planets and develops intelligence, technology, and interplanetary communication skills. Finally, it factors in the lifetime of such a civilization.

Using Drake’s equation, Verschuur calculated there may be just one other technological civilization capable of communicating with humans in the whole group of galaxies that include our Milky Way — a vanishingly small number that may explain why 30 years of scanning the skies for signs of intelligent life has come up empty.

“I’m not very optimistic,” Verschuur said.

Dimitar Sasselov, professor of astrophysics at Harvard and director of the Harvard Origins of Life Initiative, agreed with Verschuur that life is probably common in the universe. He said that he believes life is a natural “planetary phenomenon” that occurs easily on planets with the right conditions.

As for intelligent life, give it time, he said. Though it may be hard to think of it this way, at roughly 14 billion years old, the universe is quite young, he said. The heavy elements that make up planets like Earth were not available in the early universe; instead, they are formed by the stars. Enough of these materials were available to begin forming rocky planets like Earth just 7 billion or 8 billion years ago. When one considers that it took nearly 4 billion years for intelligent life to evolve on Earth, it would perhaps not be surprising if intelligence is still rare.

“It takes a long time to do this,” Sasselov said. “It may be that we are the first generation in this galaxy.”

Several speakers at the event hailed the March launch of NASA’s Kepler space telescope, which is dedicated to the search for Earth-like planets orbiting other stars. Several Harvard-Smithsonian Center for Astrophysics faculty members, including Sasselov, are investigators on the telescope mission.

Andrew Knoll describes the beginnings of life on Earth. Photograph by Stephanie Mitchell/Harvard News Office
Andrew Knoll describes the beginnings of life on Earth. Photograph by Stephanie Mitchell/Harvard News Office

Sasselov said he expects Kepler to quickly add to the 350 planets already found orbiting other stars. By the end of the summer, he said, it may have found more than a dozen “super Earths” or planets from Earth-size to just over twice Earth’s size that Sasselov expects would have the stability and conditions that would allow life to develop.

If life did develop elsewhere, Andrew Knoll, the Fisher Professor of Natural History, used the lessons of planet Earth to give an idea of what it might take to develop intelligence. Of the three major groupings of life: bacteria, archaea, and eukaryotes, only the eukaryotes developed complex life. And even among the myriad kinds of eukaryotes, complex life arose in just a few places: animals, plants, fungi, and red and brown algae. Knoll said he believes that the rise of mobility, oxygen levels, and predation, together with its need for sophisticated sensory systems, coordinated activity, and a brain, provided the first steps toward intelligence.

It has only been during the past century — a tiny fraction of Earth’s history — that humans have had the technological capacity to communicate off Earth, Knoll said. And, though Kepler may advance the search for Earth-like planets, it won’t tell us whether there’s life there, or whether there has been life there in the past.

Other speakers included J. Craig Venter, Freeman Dyson, Peter Ward, Andy Knoll, Maria Zuber, David Charbonneau, Juan Enriquez, and David Aguilar.

Source: PhysOrg

Should We Really Tell ET Our Problems?

The design etched to the Pioneer probes. The first interstellar pornography? (NASA)

[/caption]So, you have a radio transmitter and you’ve been tasked to send a message into space to try to communicate with a hypothetical alien civilization. Where do you begin? Probably high on your list is to seek out the best candidate stars to send a signal to. As we only have experience of life on Earth, it’s a pretty good idea to look for Sun-like stars, as for all you know, that is the only place where Life As We Know It™ could exist.

So now you have found the potential location of an alien civilization, what message should you send? Firstly you’d probably want to make a good impression; perhaps sending directions to Earth, a universal map with an arrow pointing at the Solar System. Secondly you might want to identify what/who you are (insert some human physiology here). And third? Perhaps you’d consider sending information about our culture, civilization, history, science; all the good stuff that makes us human.

Would it cross your mind to mention there are 23 bloody conflicts going on right now amongst our own kind? Would you think about telling our potential alien neighbours about what you just had for dinner? Would it be a good idea to tell them about the political corruption in your country, the vast poverty worldwide or the ecological damage we are doing to our own home?

In a recent article written by the director of interstellar message composition at the SETI Institute, the question about communicating honestly with ET, without sanitizing the truth, is asked. Should we really tell an alien civilization about our problems?

Communication with potential alien races is a tricky business (Ian O'Neill)
Communication with potential alien races is a tricky business (Ian O'Neill)
For five decades, the Search for Extraterrestrial Intelligence (SETI) has been scouring the skies for any signal from an intelligent alien civilization. This is a painstaking task that requires much patience and lots of ingenuity. After all, what are we looking for? Assuming extraterrestrial civilizations have worked out how to transmit radio, perhaps we could listen out for that. Unfortunately, apart from the 72 second Wow! signal in 1977, it all seems very quiet out there. If the Drake Equation is to be taken literally, the Milky Way should be teeming with life, some of which should be transmitting their greatest hits right now. There are problems with this theory, as some believe that although aliens might be transmitting, radio signals might not reach us. Perhaps then a sufficiently advanced alien race might be using powerful laser beacons or moving stars to communicate with us. Alas, nothing. Yet.

OK, so let’s turn this around. Perhaps we’ll have more luck if we start transmitting radio signals to Sun-like stars in the hope of an alien race as advanced as ourselves receiving it. This program is known as Messaging Extraterrestrial Intelligence (METI) or “Active-SETI.” But what do we say? One of the earliest messaging attempts was the plaque bolted to the side of the Pioneer spacecraft (pictured top), even though the naked human figures representing male and female caused a stir (some groups considered the naked human form interstellar pornography). Despite a few disputes about what we should be sending into space, generally the messages have been very positive, trying to portray the human race in a very positive light.

Douglas Vakoch, from the SETI Institute in Mountain View, California, disagrees with the policy of sending only positive messages into space via radio transmissions or metal plaques strapped to the sides of spaceships.

An acknowledgment of our flaws and frailties seems a more honest approach than sending a sanitised, one-sided story,” Vakoch said in a recent New Scientist column. “Honesty is a good starting point for a conversation that could last for generations.”

As the director of interstellar message composition, Vakoch obviously knows a thing or two about sending messages to our potential alien neighbours. However, the question as to whether or not we should sanitize our communications seems a little strange. Of course we should transmit the best mankind has to offer! I don’t believe sending messages of culture, science, mathematics, art and music would be setting us up for a fall. If we are indeed the new kids on the block of extraterrestrial civilizations, I think we’d need to make a great impression (depending on whether ET understands what we are trying to communicate in the first place).

The 1977 Wow! signal (SETI)
The 1977 Wow! signal (SETI)
Vakoch is keen to point out that a sufficiently advanced alien civilization is going to be savvy as to what it takes to be a a galactic race (it’s not all roses after all). If they receive a message from mankind full of positive messages, perhaps they won’t trust us. Worse still, as they get to know us, they think we were hiding our human flaws, misleading them in some way. Therefore, we need to be honest up-front. We need to send the views and opinions of as many people as possible, for good or bad, so extraterrestrial civilizations know what they are dealing with; a talented, yet flawed race.

Unfortunately, that goes against human nature. What’s the first thing you do when moving into a new neighbourhood? You might throw a house-warming party, as a way to introduce yourself to the new neighbours. You probably wouldn’t tell your neighbours about your family/money/alcohol/drug/criminal problems at the party. If you did, you might find the room emptying very quickly. It’s not that you are being dishonest, you’re trying to gain their first-impression trust and interest. This principal holds true for companies trying to sell a product (I have yet to have a doorstep sales person telling me his encyclopaedia collection is actually useless when the world has Wikipedia) and to countries forming new diplomatic ties. We know there’s more to the story than just first impressions, but first impressions are the bonds that help develop the relationship in the future.

Assimilation could be ET's solution to human problems
Assimilation could be ET's solution to human problems
So going back to being honest with messaging alien civilizations, if we send “the truth” about our race, we would actually be doing ourselves a disservice. What if the receiving alien civilization doesn’t want to be associated with us as we are considered too aggressive, cruel, greedy or weird?

We can’t second-guess how an extraterrestrial civilization is going to respond to us, there is no precedent of alien communications, so perhaps we should take the “sanitized” approach. Positive information is probably enough information; too much information could turn us into interstellar outcasts before we’ve even had a chance to receive a message from another star. (I thought it was a little too quiet out there, perhaps they received our commercial TV signals.)

And if the advanced alien race deems us “not worthy” on account of the mixed signals we are sending out, they might turn hostile sooner rather than later